Synthetic profile analysis of the observed (0,0) Swan band of Comet Halley

Details Synthetic profile analysis of the observed (0,0) Swan band of Comet Halley Synthetic profile analysis of the observed (0,0) Swan band of Comet Halley

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...373..266k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 373, May 20, 1991, p. 266-270.

Astronomy and Astrophysics

Astrophysics

5

Carbon, Halley'S Comet, Molecular Spectra, Swan Bands, Astronomical Models, Spectrum Analysis, Time Dependence

Scientific paper

The time-dependent rotational population distribution for the (0,0) band of the Swan system was carried out. These population distributions are used to calculate the synthetic spectra over the wavelength region 5165-5132 A for comparing with the excellent spectra of Lambert et al. (1990) for Comet Halley. The synthetic spectra for the rotational population distribution corresponding to a time interval of about 8000 sec gives a good fit to the observed spectra over the whole special region. This seems to indicate that the level population does not appear to have reached the steady state values.

Affiliated with

Also associated with

No associations

Rating

Synthetic profile analysis of the observed (0,0) Swan band of Comet Halley does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Synthetic profile analysis of the observed (0,0) Swan band of Comet Halley, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Synthetic profile analysis of the observed (0,0) Swan band of Comet Halley will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1036970